英语词汇“chromosphere”的意思、用法、释义、翻译、读音、例句、短语、词组-英语词典

是什么意思

色球；

英英释义

chromosphere[ 'kr?um?,sfi? ]

n.a gaseous layer of the sun's atmosphere (extending from the photosphere to the corona) that is visible during a total eclipse of the sun

学习怎么用

双语例句

用作名词(n.)

It is difficult to photograph the actual chromosphere.
拍摄实际的色球层很困难。
The rest escapes as sound waves, mechanical vibrations that heat the chromosphere, the middle layer of the sun's atmosphere.
其余部分则以声波即机械振动的形式散逸，它们加热了太阳大气的中间一层，即色球层。

权威例句

Mass and Energy Flow in the Solar Chromosphere and Corona
On the Structure of the Solar Corona and Chromosphere
Dynamics of the solar chromosphere. I - Long-period network oscillations
Structure of the Solar Chromosphere. Basic Computations and Summary of the Results
The Heating of the Solar Chromosphere, Plages, and Corona by Magnetohydrodynamic Waves.
Structure of the solar chromosphere. III - Models of the EUV brightness components of the quiet-sun
Structure of the solar chromosphere. II - The underlying photosphere and temperature-minimum region
Motion of magnetic flux tubes in the solar convection zone and chromosphere
Flare Loop Radiative Hydrodynamics - Part Seven - Dynamics of the Thick Target Heated Chromosphere
Numerical simulation of the three-dimensional structure and dynamics of the non-magnetic solar chromosphere

单词	chromosphere
释义	chromosphere 听听怎么读英 ['kr??m?sf??] 美 [?krom??sf?r] 是什么意思 n. 色球；英英释义 chromosphere[ 'kr?um?,sfi? ] n.a gaseous layer of the sun's atmosphere (extending from the photosphere to the corona) that is visible during a total eclipse of the sun 学习怎么用双语例句用作名词(n.) It is difficult to photograph the actual chromosphere. 拍摄实际的色球层很困难。 The rest escapes as sound waves, mechanical vibrations that heat the chromosphere, the middle layer of the sun's atmosphere. 其余部分则以声波即机械振动的形式散逸，它们加热了太阳大气的中间一层，即色球层。权威例句 Mass and Energy Flow in the Solar Chromosphere and Corona On the Structure of the Solar Corona and Chromosphere Dynamics of the solar chromosphere. I - Long-period network oscillations Structure of the Solar Chromosphere. Basic Computations and Summary of the Results The Heating of the Solar Chromosphere, Plages, and Corona by Magnetohydrodynamic Waves. Structure of the solar chromosphere. III - Models of the EUV brightness components of the quiet-sun Structure of the solar chromosphere. II - The underlying photosphere and temperature-minimum region Motion of magnetic flux tubes in the solar convection zone and chromosphere Flare Loop Radiative Hydrodynamics - Part Seven - Dynamics of the Thick Target Heated Chromosphere Numerical simulation of the three-dimensional structure and dynamics of the non-magnetic solar chromosphere
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